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Fig. 10


MHI vs. MH2 deficiencies (left) and MHI vs. LFIR deficiencies (right) for spiral galaxies (T ≥ 1). The red lines show Def(MHI) = 0, Def(MH2) = 0 and Def(LFIR) = 0, and the dashed lines give Def(MH2) = 0.75, separating low and highly HI-deficient galaxies in our analysis. Red symbols denote upper limits in MH2 or LFIR.

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